YNAO OpenIR  > 高能天体物理研究组
THE FIRST FERMI LAT SUPERNOVA REMNANT CATALOG
Acero, F.1; Ackermann, M.2; Ajello, M.3; Baldini, L.4,5,6,7; Ballet, J.1; Barbiellini, G.8,9; Bastieri, D.10,11; Bellazzini, R.12; Bissaldi, E.13; Blandford, R. D.6,7; Bloom, E. D.6,7; Bonino, R.14,15; Bottacini, E.6,7; Brandt, T. J.16; Bregeon, J.17; Bruel, P.18; Buehler, R.2; Buson, S.10,11; Caliandro, G. A.6,7,19; Cameron, R. A.6,7; Caputo, R.20,21; Caragiulo, M.13; Caraveo, P. A.22; Casandjian, J. M.1; Cavazzuti, E.23; Cecchi, C.24,25; Chekhtman, A.26,27; Chiang, J.6,7; Chiaro, G.11; Ciprini, S.23,24,28; Claus, R.6,7; Cohen, J. M.16,29,30; Cohen-Tanugi, J.17; Cominsky, L. R.31; Condon, B.32; Conrad, J.33,34,35; Cutini, S.23,24,28; D'Ammando, F.36,37; de Angelis, A.38,39; de Palma, F.13,40; Desiante, R.14,41; Digel, S. W.6,7; Di Venere, L.42,43; Drell, P. S.6,7; Drlica-Wagner, A.44; Favuzzi, C.13,42,43; Ferrara, E. C.16; Franckowiak, A.6,7; Fukazawa, Y.45; Funk, S.46; Fusco, P.13,42,43; Gargano, F.13; Gasparrini, D.23,24,28; Giglietto, N.13,42,43; Giommi, P.23; Giordano, F.13,42,43; Giroletti, M.36; Glanzman, T.6,7; Godfrey, G.6,7; Gomez-Vargas, G. A.47,48; Grenier, I. A.1; Grondin, M. -H.32; Guillemot, L.49,50; Guiriec, S.16,90; Gustafsson, M.51; Hadasch, D.52,53; Harding, A. K.16; Hayashida, M.54; Hays, E.16; Hewitt, J. W.55; Hill, A. B.6,7,56; Horan, D.18; Hou X(侯贤)57,58; Iafrate, G.8,59; Jogler, T.6,7; Johannesson, G.60; Johnson, A. S.6,7; Kamae, T.61; Katagiri, H.62; Kataoka, J.63; Katsuta, J.45; Kerr, M.64; Knodlseder, J.65,66; Kocevski, D.16; Kuss, M.12; Laffon, H.32; Lande, J.67; Larsson, S.34,68; Latronico, L.14; Lemoine-Goumard, M.32; Li, J.69; Li, L.34,68; Longo, F.8,9; Loparco, F.13,42,43; Lovellette, M. N.70; Lubrano, P.24,25; Magill, J.29,30; Maldera, S.14; Marelli, M.22; Mayer, M.2; Mazziotta, M. N.13; Michelson, P. F.6,7; Mitthumsiri, W.71; Mizuno, T.72; Moiseev, A. A.29,30,73,74; Monzani, M. E.6,7; Moretti, E.75; Morselli, A.47; Moskalenko, I. V.6,7; Murgia, S.76; Nemmen, R.77; Nuss, E.17; Ohsugi, T.72; Omodei, N.6,7; Orienti, M.36; Orlando, E.6,7; Ormes, J. F.78; Paneque, D.6,7,75; Perkins, J. S.16; Pesce-Rollins, M.6,7,12; Petrosian, V.6,7; Piron, F.17; Pivato, G.12; Porter, T. A.6,7; Raino, S.14,44; Rando, R.10,11; Razzano, M.12; Razzaque, S.79; Reimer, A.6,7,52,53; Reimer, O.6,7,52,53; Renaud, M.17; Reposeur, T.32; Rousseau, R.80; Parkinson, P. M. Saz20,21,81; Schmid, J.1; Schulz, A.2; Sgro, C.12; Siskind, E. J.82; Spada, F.12; Spandre, G.12; Spinelli, P.13,42,43; Strong, A. W.83; Suson, D. J.84; Tajima, H.6,7,85; Takahashi, H.45; Tanaka, T.86; Thayer, J. B.6,7; Thompson, D. J.16; Tibaldo, L.6,7; Tibolla, O.87; Torres, D. F.69,88; Tosti, G.24,25; Troja, E.16,29,30; Uchiyama, Y.89; Vianello, G.6,7; Wells, B.20,21; Wood, K. S.70; Wood, M.6,7; Yassine, M.17; den Hartog, P. R.6,7,90; Zimmer, S.33,34; de Palma, F
Source PublicationASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
2016-05-01
Volume224Issue:1
DOI10.3847/0067-0049/224/1/8
Contribution Rank第49完成单位
Indexed BySCI
KeywordAcceleration Of Particles Catalogs Cosmic Rays Gamma-rays: Ism Ism: Supernova Remnants Radiation Mechanisms: Nonthermal
Abstract

To uniformly determine the properties of supernova remnants (SNRs) at high energies, we have developed the first systematic survey at energies from 1 to 100 GeV using data from the Fermi Large Area Telescope (LAT). Based on the spatial overlap of sources detected at GeV energies with SNRs known from radio surveys, we classify 30 sources as likely GeV SNRs. We also report 14 marginal associations and 245 flux upper limits. A mock catalog in which the positions of known remnants are scrambled in Galactic longitude allows us to determine an upper limit of 22% on the number of GeV candidates falsely identified as SNRs. We have also developed a method to estimate spectral and spatial systematic errors arising from the diffuse interstellar emission model, a key component of all Galactic Fermi LAT analyses. By studying remnants uniformly in aggregate, we measure the GeV properties common to these objects and provide a crucial context for the detailed modeling of individual SNRs. Combining our GeV results with multiwavelength (MW) data, including radio, X-ray, and TeV, we demonstrate the need for improvements to previously sufficient, simple models describing the GeV and radio emission from these objects. We model the GeV and MW emission from SNRs in aggregate to constrain their maximal contribution to observed Galactic cosmic rays.

Funding ProjectIstituto Nazionale di Astrofisica in Italy ; Centre National d'Etudes Spatiales in France
Funding OrganizationIstituto Nazionale di Astrofisica in Italy ; Centre National d'Etudes Spatiales in France
Language英语
Subject Area天文学 ; 天体物理学 ; 高能天体物理学 ; 实测天体物理学
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeArticle
PublisherIOP PUBLISHING LTD
Publication PlaceTEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0067-0049
URL查看原文
WOS IDWOS:000377050200008
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordLARGE-AREA TELESCOPE ; GAMMA-RAY EMISSION ; VERY-HIGH-ENERGY ; PULSAR-WIND NEBULA ; DIFFUSIVE SHOCK ACCELERATION ; HARD X-RAY ; MHZ MASER EMISSION ; XMM-NEWTON OBSERVATIONS ; GALACTIC PLANE SURVEY ; HIGH MAGNETIC-FIELD
Citation statistics
Cited Times:78[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/9604
Collection高能天体物理研究组
中国科学院天体结构与演化重点实验室
Corresponding Authorde Palma, F.; de Palma, F
Affiliation1.Univ Paris Diderot, CEA Saclay, Lab AIM, CEA,IRFU,CNRS,Serv Astrophys, F-91191 Gif Sur Yvette, France
2.Deutsch Elektronen Synchrotron DESY, D-15738 Zeuthen, Germany
3.Clemson Univ, Dept Phys & Astron, Kinard Lab Phys, Clemson, SC 29634 USA
4.Univ Pisa, I-56127 Pisa, Italy
5.Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy
6.Stanford Univ, Dept Phys, WW Hansen Expt Phys Lab, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA
7.Stanford Univ, SLAC Natl Accelerator Lab, Stanford, CA 94305 USA
8.Ist Nazl Fis Nucl, Sez Trieste, I-34127 Trieste, Italy
9.Univ Trieste, Dipartimento Fis, I-34127 Trieste, Italy
10.Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy
11.Univ Padua, Dipartimento Fis & Astron G Galilei, I-35131 Padua, Italy
12.Ist Nazl Fis Nucl, I-56127 Pisa, Italy
13.Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy
14.Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy
15.Ist Nazl Fis Nucl, Dipartimento Fis Gen Amadeo Avogadro, I-10125 Turin, Italy
16.NASA, Goddard Space Flight Ctr, Code 661, Greenbelt, MD 20771 USA
17.Univ Montpellier, CNRS, IN2P3, Lab Univers & Particules Montpellier, F-34059 Montpellier, France
18.Ecole Polytech, CNRS, IN2P3, Lab Leprince Ringuet, F-91128 Palaiseau, France
19.CIFS, I-10133 Turin, Italy
20.Univ Calif Santa Cruz, Dept Phys, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA
21.Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA
22.INAF Ist Astrofis Spaziale & Fis Cosm, I-20133 Milan, Italy
23.ASI Sci Data Ctr, I-20133 Milan, Italy
24.Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy
25.Univ Perugia, Dipartimento Fis, I-06123 Perugia, Italy
26.George Mason Univ, Coll Sci, Fairfax, VA 22030 USA
27.Naval Res Lab, Washington, DC 20375 USA
28.INAF Osservatorio Astron Roma, I-00040 Monte Porzio Catone, Roma, Italy
29.Univ Maryland, Dept Phys, College Pk, MD 20742 USA
30.Univ Maryland, Dept Astron, College Pk, MD 20742 USA
31.Sonoma State Univ, Dept Phys & Astron, Rohnert Pk, CA 94928 USA
32.Univ Bordeaux 1, CNRS, IN2P3, Ctr Etud Nucl Bordeaux Gradignan, BP120, F-33175 Gradignan, France
33.Stockholm Univ, Dept Phys, AlbaNova, SE-10691 Stockholm, Sweden
34.AlbaNova, Oskar Klein Ctr Cosmoparticle Phys, SE-10691 Stockholm, Sweden
35.Royal Swedish Acad Sci, Box 50005, SE-10405 Stockholm, Sweden
36.INAF Ist Radioastron, I-40129 Bologna, Italy
37.Univ Bologna, Dipartimento Astron, I-40127 Bologna, Italy
38.Univ Udine, Dipartimento Fis, I-33100 Udine, Italy
39.Ist Nazl Fis Nucl, Sez Trieste, Grp Coll Udine, I-33100 Udine, Italy
40.Univ Telemat Pegaso, Piazza Trieste & Trento 48, I-80132 Naples, Italy
41.Univ Udine, I-33100 Udine, Italy
42.Univ Bari, Dipartimento Fis M Merlin, I-70126 Bari, Italy
43.Politecn Bari, I-70126 Bari, Italy
44.Fermilab Natl Accelerator Lab, Ctr Particle Astrophys, Batavia, IL 60510 USA
45.Hiroshima Univ, Dept Phys Sci, Higashihiroshima, Hiroshima 7398526, Japan
46.Erlangen Ctr Astroparticle Phys, D-91058 Erlangen, Germany
47.Ist Nazl Fis Nucl, Sez Roma Tor Vergata, I-00133 Rome, Italy
48.Pontificia Univ Catolica Chile, Dept Fis, Ave Vicuna Mackenna 4860, Santiago, Chile
49.Univ Orleans, Lab Phys & Chim Environm & Espace, CNRS, F-45071 Orleans 02, France
50.Observ Paris, CNRS, INSU, Stn Radioastron Nancay, F-18330 Nancay, France
51.Univ Gottingen, Inst Theoret Phys, Fac Phys, Friedrich Hund Pl 1, D-37077 Gottingen, Germany
52.Leopold Fanzens Univ Innsbruck, Inst Astro & Teilchenphys, A-6020 Innsbruck, Austria
53.Leopold Fanzens Univ Innsbruck, Inst Theoret Phys, A-6020 Innsbruck, Austria
54.Univ Tokyo, Inst Cosm Ray Res, 5-1-5 Kashiwanoha, Kashiwa, Chiba 2778582, Japan
55.Univ N Florida, Dept Phys, 1 UNF Dr, Jacksonville, FL 32224 USA
56.Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, Hants, England
57.Chinese Acad Sci, Yunnan Observ, Kunming 650216, Peoples R China
58.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650216, Peoples R China
59.Osserv Astron Trieste, Ist Nazl Astrofis, I-34143 Trieste, Italy
60.Univ Iceland, Inst Sci, Dunhaga 3, IS-107 Reykjavik, Iceland
61.Univ Tokyo, Grad Sch Sci, Dept Phys, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan
62.Ibaraki Univ, Coll Sci, 2-1-1 Bunkyo, Mito, Ibaraki 3108512, Japan
63.Waseda Univ, Res Inst Sci & Engn, Shinjuku Ku, 3-4-1 Okubo, Tokyo 1698555, Japan
64.CSIRO Astron & Space Sci, Australia Telescope Natl Facil, Epping, NSW 1710, Australia
65.CNRS, IRAP, F-31028 Toulouse 4, France
66.Univ Toulouse, GAHEC, UPS OMP, IRAP, Toulouse, France
67.Twitter Inc, 1355 Market St 900, San Francisco, CA 94103 USA
68.KTH Royal Inst Technol, Dept Phys, AlbaNova, SE-10691 Stockholm, Sweden
69.CSIC, Inst Space Sci IEEC, Campus UAB, E-08193 Barcelona, Spain
70.Naval Res Lab, Div Space Sci, Washington, DC 20375 USA
71.Mahidol Univ, Dept Phys, Fac Sci, Bangkok 10400, Thailand
72.Hiroshima Univ, Hiroshima Astrophys Sci Ctr, Hiroshima 7398526, Japan
73.CRESST, Greenbelt, MD 20771 USA
74.NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
75.Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany
76.Univ Calif Irvine, Dept Phys & Astron, Ctr Cosmol, Irvine, CA 92697 USA
77.Univ Sao Paulo, Inst Astron Geofis & Cincias Atmosfer, Rua Matdo 1226, BR-05508090 Sao Paulo, SP, Brazil
78.Univ Denver, Dept Phys & Astron, Denver, CO 80208 USA
79.Univ Johannesburg, Dept Phys, POB 524, ZA-2006 Auckland Pk, South Africa
80.Lycee Fresnel, Paris, France
81.Univ Hong Kong, Dept Phys, Pokfulam Rd, Hong Kong, Hong Kong, Peoples R China
82.NYCB Real Time Comp Inc, Lattingtown, NY 11560 USA
83.Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
84.Purdue Univ Calumet, Dept Chem & Phys, Hammond, IN 46323 USA
85.Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan
86.Kyoto Univ, Grad Sch Sci, Dept Phys, Kyoto, Japan
87.Univ Autonoma Chiapas UNACH, MCTP, Carretera Emiliano Zapata Km 4, Tuxtla Gutierrez 29050, Chiapas, Mexico
88.ICREA, Barcelona, Spain
89.3-34-1 Nishi Ikebukuro,Toshima Ku, Tokyo 1718501, Japan
90.HAL24K Data Intelligence Labs, Barbara Strozzilaan, NL-1083 HN Amsterdam, Netherlands
Recommended Citation
GB/T 7714
Acero, F.,Ackermann, M.,Ajello, M.,et al. THE FIRST FERMI LAT SUPERNOVA REMNANT CATALOG[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2016,224(1).
APA Acero, F..,Ackermann, M..,Ajello, M..,Baldini, L..,Ballet, J..,...&de Palma, F.(2016).THE FIRST FERMI LAT SUPERNOVA REMNANT CATALOG.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,224(1).
MLA Acero, F.,et al."THE FIRST FERMI LAT SUPERNOVA REMNANT CATALOG".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 224.1(2016).
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